Titlebook: Neutron Stars and Their Birth Events; Wolfgang Kundt Book 1990 Kluwer Academic Publishers 1990 Accretion.Population.Supernova.accretion di

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Prophylaxis

內(nèi)向者

Functional

Millisecond Pulsars: A New Population of Gamma Ray Sources?,heir acceleration, and the observed gamma ray emission may be from the same region, or nearby regions of the magnetosphere. Thus, in an indirect way, the pulsed gamma rays are telling us something about the location of the particle accelerator.

phlegm

2D Relativistic Pulsar Winds From Rapidly Rotating Neutron Stars,he hot wind equation for the pair plasma and the relativistic Grad-Schlüter-Shafranov (GSS) equation for the magnetic flux function. The structure of the solutions for the hot pair wind equation is discussed. We also show how self-consistent axisymmetric MHD magnetospheres can be constructed by simu

用肘

Book 1990o the proceedings. Several lecturers speak of ‘magnetic-field decay‘ in neutron stars, of the ‘recycling‘ of old pulsars, and of ‘a(chǎn)ccretion-induced collapse‘ of white dwarfs as though such processes were textbook knowledge. Terms and abbreviations like RPSR (=recycled pulsar), spinup line, AIC, and

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